This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 2036 and 2200 | ||||
|---|---|---|---|---|
 July 23, 2036 (Saros 117) |
 June 23, 2047 (Saros 118) |
 May 22, 2058 (Saros 119) |
 April 21, 2069 (Saros 120) |
 March 21, 2080 (Saros 121) |
 February 18, 2091 (Saros 122) |
 January 19, 2102 (Saros 123) |
 December 19, 2112 (Saros 124) |
 November 18, 2123 (Saros 125) |
 October 17, 2134 (Saros 126) |
 September 16, 2145 (Saros 127) |
 August 16, 2156 (Saros 128) |
 July 16, 2167 (Saros 129) |
 June 16, 2178 (Saros 130) |
 May 15, 2189 (Saros 131) |
 April 14, 2200 (Saros 132) | ||||